Measuring High Moments of Galaxy Angular Distribution in the First Look Survey using Infrared Array Camera

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dc.creatorFang, Fan
dc.creatorTeam, the FLS
dc.date2005-03-03
dc.date.accessioned2026-07-07T02:17:08Z
dc.date.available2026-07-07T02:17:08Z
dc.descriptionWe present the results of using three methods, the probability distribution function, the Renyi information, and the multi-fractals, to measure the high moments of galaxy angular distribution in the Infrared Array Camera data of the Spitzer First Look Survey. This is the first time that Renyi information is explicitly used to describe the large-scale galaxy spatial distribution, and our galaxy samples are also the first of the kind in their wavelengths and sensitivities.
dc.identifierhttps://arxiv.org/abs/astro-ph/0503084
dc.identifierhttp://arxiv.org/abs/astro-ph/0503084
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9064
dc.subjectAstrophysics
dc.subjectData Analysis, Statistics and Probability
dc.titleMeasuring High Moments of Galaxy Angular Distribution in the First Look Survey using Infrared Array Camera
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